会议论文详细信息
11th International Spring Seminar on Nuclear Physics: Shell Model and Nuclear Structure – achievements of the past two decades | |
Shell model studies for nuclear astrophysics | |
Langanke, K.^1,2,3 ; Martínez-Pinedo, G.^1,2 | |
GSI Helmholtzzentrum für Schwerionenforschung, Planckstr. 1, Darmstadt | |
64291, Germany^1 | |
Institut für Kernphysik, TU Darmstadt, Schlossgartenstr. 9, Darmstadt | |
64291, Germany^2 | |
Frankfurt Institute for Advanced Studies, Ruth-Moufang-Str. 1, Frankfurt | |
60438, Germany^3 | |
关键词: Astrophysical objects; Core collapse supernovae; Electron capture; Neutron number; Neutron-rich nuclei; Nuclear astro-physics; Shell models; Supernova neutrinos; | |
Others : https://iopscience.iop.org/article/10.1088/1742-6596/580/1/012033/pdf DOI : 10.1088/1742-6596/580/1/012033 |
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来源: IOP | |
【 摘 要 】
Shell model studies have contributed in recent years significantly to improve nuclear input required in simulations of the dynamics of astrophysical objects and their associated nucleosynthesis. This manuscript highlights a few examples like electron capture rates of importance for the evolution of core-collapse supernovae and the nucleosynthesis in thermonuclear supernovae, neutrino-nucleus cross sections with relevance to the supernova neutrino spectra and finally half lives of neutron-rich nuclei with magic neutron numbers which serve as waiting points in the mass flow of the astrophysical r-process.
【 预 览 】
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